A spectroscopic study of the optical counterparts of three X-ray bursters

Details A spectroscopic study of the optical counterparts of three X-ray bursters A spectroscopic study of the optical counterparts of three X-ray bursters

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234..556c&link_type=abstract

Astrophysical Journal, Part 1, vol. 234, Dec. 1, 1979, p. 556-565.

Astronomy and Astrophysics

Astronomy

47

Binary Stars, Companion Stars, Stellar Spectra, X Ray Sources, X Ray Stars, Balmer Series, Emission Spectra, Galactic Bulge, Main Sequence Stars, Spectral Line Width

Scientific paper

One of the major puzzles in galactic X-ray astronomy is the nature of the galactic bulge sources in general and the X-ray burst sources in particular. The answer to this puzzle is likely to come from studies of the faint blue optical counterparts which have been identified with several of these sources. As part of such a study, some results of a detailed investigation of the spectroscopic properties of the optical counterparts to three X-ray bursters - 4U 1735-44, 4U 1636-53, and MXB 1659-29.

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